THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE
2014 ◽
Vol 23
(02)
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pp. 1450013
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Keyword(s):
The Core
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In this paper, we investigate the physics of a radiating star undergoing dissipative collapse in the form of a radial heat flux. Our treatment clearly demonstrates how the presence of shear affects the collapse process; we are in a position to contrast the physical features of the collapsing sphere in the presence of shear with the shear-free case. By employing a causal heat transport equation of the Maxwell–Cattaneo form we show that the shear leads to an enhancement of the core temperature thus emphasizing that relaxational effects cannot be ignored when the star leaves hydrostatic equilibrium.
2016 ◽
Vol 26
(07)
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pp. 1750065
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2020 ◽
Vol 35
(20)
◽
pp. 2050164
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2021 ◽
Vol 81
(2)
◽
Keyword(s):
2013 ◽
Vol 22
(07)
◽
pp. 1350049
◽
Keyword(s):
1981 ◽
pp. 19-28
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Keyword(s):
2018 ◽
Vol 50
(2)
◽
pp. 1-13
2020 ◽
Vol 63
(2)
◽
pp. 46-62